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Optically Thick Steady-State Accretion Disk Model Analyses of Three Dwarf Novae in Outburst
Optically Thick Steady-State Accretion Disk Model Analyses of Three Dwarf Novae in Outburst
2005
S. G. Stegman
Edward M. Sion
Keywords:
White dwarf
Intermediate polar
Accretion disc
Steady state
Astronomy
Cataclysmic variable star
Astrophysics
Physics
Correction
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